CWNU 1130

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C3
N_50
r_50
CB 35 11.8
Summary

CWNU 1130 is a poorly populated, moderately dense object of low C3 quality. It is located at a relatively close distance from the Sun, above the mid-plane. It was recently reported in the literature.

This object shares a significant percentage of members with a later reported entry.

Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2022) 49.062 60.591 0.934 0.335 0.676
           
UCC 49.037 60.602 0.932 0.34 0.675 -24.929
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1130 UCC

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Fundamental parameters

Reference Values
He et al. (2022) A0=1.85, logAge=7.15

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Theia 1740 65.7 49.25 60.54 0.94 0.34 0.64 -13.46 0.04